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Jezero on the edge of the Isidis basin. Jezero [a] (ICAO: JZRO) is a crater on Mars in the Syrtis Major quadrangle, [3] about 45.0 km (28.0 mi) in diameter. Thought to have once been flooded with water, the crater contains a fan-delta deposit rich in clays. [4]
Octavia E. Butler Landing is the February 18, 2021, landing site of the Mars 2020 Perseverance rover within Jezero crater on planet Mars. On March 5, 2021, NASA named the site for the American science fiction author, Octavia E. Butler, who died on February 24, 2006. The Mars landing took place nearly 15 years to the day after her death.
The series of valleys leading into the delta "drain" an area of approximately 4000 km 2. The surface area of the delta is 115 km 2, measuring 13 km by 11 km. The delta was discovered from images acquired by the Mars Global Surveyor in 2003, operated Malin Space Science Systems. Eberswalde delta has six lobes and is about 100 meters thick. [6]
These formations are: Pancake Delta, Western Delta, Farah Vallis delta and the Peace Vallis Fan. [117] In a press conference on 8 December 2014, Mars scientists discussed observations by Curiosity rover that show Mars' Mount Sharp was built by sediments deposited in a large lake bed over tens of millions of years. This finding suggests the ...
In particular, precipitation induced surface runoff and groundwater seepage resulted in the formation of fluvial landforms, i.e., dense valley networks, [2] broad and elongated valleys, delta deposits, alluvial fans, open-basin paleolakes and coastlines. Crater size - frequency distribution measurements ("crater counting") revealed that the ...
Reull Vallis with lineated floor deposits. Location is Hellas quadrangle. Glacier-like features on Mars are known variously as viscous flow features, [290] Martian flow features, lobate debris aprons, [58] or lineated valley fill, [54] depending on the form of the feature, its location, the landforms it is associated with, and the author ...
Rocks on Mars have been found to frequently occur as layers, called strata, in many different places. Columbus Crater is one of many craters that contain layers. Rock can form layers in a variety of ways. Volcanoes, wind, or water can produce layers. [83] Many places on Mars show rocks arranged in layers.
This is a partial list of named channel structures on Mars claimed as outflow channels in the literature, largely following The Surface of Mars by Carr. The channels tend to cluster in certain regions on the Martian surface, often associated with volcanic provinces, and the list reflects this.